Relativistic Processes and the Internal Structure of Neutron Stars

TL;DR

This paper reviews models of dense neutron star interiors and their observable relativistic phenomena, focusing on neutron matter modeling and crust properties using a two-fluid approach.

Contribution

It introduces a comprehensive review of internal composition models and presents new insights into crust properties with a two-fluid model approach.

Findings

Neutron star models align with relativistic observational data

Crust properties are characterized by a two-fluid model

Enhanced understanding of dense matter in neutron stars

Abstract

Models for the internal composition of Dense Compact Stars are reviewed as well as macroscopic properties derived by observations of relativistic processes. Modeling of pure neutron matter Neutron Stars is presented and crust properties are studied by means of a two fluid model.